The total intensity image of Cygnus A shows the expected combination of compact and extended structure that has been previously observed at low radio frequencies [1]}, [2]}, [3]}. For the lobe, which is to the west of the central core, the two main hotspots have been detected, with hotspot A at the edge of the lobe being the brighter of the two, whereas the fainter hotspot B is embedded within the lobe emission. The counter-lobe, which is to the east of the central core, shows a great deal of structure that includes hotspot D and enhanced emission around the edge of the counter-lobe. The back-flow and plume emission between the lobe and counter-lobe have also been clearly detected.
